- Research Article
- Open Access

# Hardware Architecture for Pattern Recognition in Gamma-Ray Experiment

- Sonia Khatchadourian
^{1}Email author, - Jean-Christophe Prévotet
^{2}and - Lounis Kessal
^{1}

**2009**:737689

https://doi.org/10.1155/2009/737689

© Sonia Khatchadourian et al. 2009

**Received:**19 March 2009**Accepted:**21 July 2009**Published:**10 September 2009

## Abstract

The HESS project has been running successfully for seven years. In order to take into account the sensitivity increase of the entire project in its second phase, a new trigger scheme is proposed. This trigger is based on a neural system that extracts the interesting features of the incoming images and rejects the background more efficiently than classical solutions. In this article, we present the basic principles of the algorithms as well as their hardware implementation in FPGAs (Field Programmable Gate Arrays).

## Keywords

- Hardware Implementation
- Zernike Moment
- Trigger System
- Geometric Moment
- Trigger Scheme

## 1. Introduction

For many years, the study of gamma photons have led scientists to understand more deeply the complex processes that occur in the Universe, for example, remnants of supernova explosions, cosmic rays interactions with interstellar gas, and so forth. In the 1960s, it has finally been possible to develop efficient measuring instruments to detect gamma-ray emissions, thus enabling to validate the theoretical concepts. Most of these instruments were built in order to identify the direction of gammas rays. Since gamma photons are not deflected by interstellar magnetic fields, it becomes possible to determine the position of the source accurately. In this context, Imaging Atmospheric Cherenkov Telescopes constitute the most sensitive technique for the observation of high-energy gamma-rays. Such telescopes provide a large effective collection area and achieve excellent angular and energy resolution for detailed studies of cosmic objects. The technique relies upon Cherenkov light produced by the secondary particles once the gamma-ray interacts with the atmosphere at about 10 km of altitude. It results a shower of secondary particles, that also may interact with the atmosphere producing other particles according to well-known physical rules. By detecting shower particles (electrons, muons, protons), it is then possible to reconstruct the initial event and determine the precise location of a source within the Universe.

In order to determine the nature of the shower, it is important to analyze its composition, that is, determine the types of particles that have been produced during the interaction with the atmosphere. This is performed by studying the different images that are collected by the telescopes and that are generally representative of the particle type. For example, gamma-ray showers usually have thin, high-density structures. On the other hand, protons are quite broad with low density.

The major problem in these experiments is that the number of images to be collected is generally huge and the complete storage of all events is impossible. This is mainly due to the fact that data-storage capacity is limited and that it is impossible to keep track of all incoming images for off-line analysis.

In order to circumvent this issue, a trigger system is often used to select the events that are interesting (from a physicist's point of view). This processing must be performed in real time and is very tightly constrained in terms of latency since it is compatible with the data acquisition rate of the cameras. The role of such triggering system is to rapidly decide whether an event is to be recorded for further studies or rejected by the system.

The organization of this paper is given as follows: the context of our work is presented in Section 2. Section 3 describes the algorithms that are envisaged in order to build a new trigger system. Considerations on hardware implementations are then provided in Section 4 and Section 5 describes the results in terms of timing and resource usage.

## 2. The HESS Project

The High-Energy Stereoscopic System (HESS) is a system of imaging Cherenkov telescopes that strive to investigate cosmic gamma rays in the 100 GeV to 100 TeV energy range [1]. It is located in Namibia at an altitude of 1800 m where the optical quality is excellent. The Phase-I of this project went into operation in Summer 2002 and consists of four Large Cherenkov Telescopes (LCT), each of 107 mirror area in order to provide a good stereoscopic viewing of the air showers. The telescopes are arranged on a square of 120 m sides, enabling thus to optimize the collection area.

The cameras of the four telescopes serve to capture and record the Cherenkov images of air showers. They have excellent resolution since the pixel size is very small: each camera is equipped of 960 photomultiplier tubes (PMTs) that are assimilated to pixels.

An efficient trigger scheme has also been designed in order to reject background such as the light of the night sky that interferes with measurements. Next sections describe both phases of the project in terms of triggering issues.

### 2.1. Phase-I

The trigger system of the HESS Phase-I project is devised in order to make use of the stereoscopic approach: simultaneous observation of interesting images must be required in order to store a specific event [2]. This coincidence requirement reduces the rate of background events, that is, events that may be assimilated to night sky noise. It is composed of two separate levels (L1 and the central trigger).

At the first level, a basic threshold is applied on signals collected by the camera. A trigger occurs if the signals in pixels within a 64-pixel sector of the camera exceed a value of photoelectrons. This enables to get rid of isolated pixels and thus to eliminate the noise. The pixel signals are sampled using 1 GHZ Analogue Ring Samplers (ARSs) [3] with a ring buffer depth of 128 cells. Following a camera trigger, the ring buffer is stopped and its content is digitized, summed and written in an FPGA buffer. After read-out, the camera is ready for the next event, and further processing may be performed including the transmission of data via optical cable to the PC processor farm located in the control building.

### 2.2. Phase-II

Since its inception in 2002, the HESS project keeps on delivering very significant results. In this very promising context, researchers of the collaboration have decided to improve the initial project by adding a new Very Large Central Telescope (VLCT) in the middle of the four existing ones. This new telescope should permit to increase the sensitivity of the global system as well as improving resolution for high-energy particles. It is composed of 2048 pixels which represent the energy of the incident event.

Considering the new approach, the quantity of data to be collected would drastically increase, and it becomes necessary to build a new trigger system in order to be compatible with the new requirements of the project.

One of the most challenging objectives of the HESS project is to detect particles which energy are below 50 GeV. In this energy range, it is not conceivable to use all telescopes (since the smallest ones cannot trigger), and only the fifth telescope may be used in a monoscopic mode.

## 3. The HESS2 L2 Triggering System

In order to cope with the new performances of the HESS Phase-II system, an efficient L2 trigger scheme is currently being built. Like all triggers, it aims to provide a decision regarding the interest of a particular event. In this context, two parallel studies have been led in order to identify the best algorithms to implement at that level. The first study relied on the Hillas parameters which are seen as a classical solution in astrophysics pattern recognition. The second study that has been envisaged is to use pattern recognition tools such as neural networks associated with an intelligent preprocessing. Both approaches are described in the next sections.

### 3.1. The First Approach

#### 3.1.1. Hillas Parameters

#### 3.1.2. The Classifier

In this first approach, the classifier consists in applying thresholds on the hillas parameters (or a combination of these parameters) computed on the incoming images in order to distinguish gamma signatures between all collected images. One of the best parameters that have been identified as a good discriminator is the Center of Gravity ( ). This parameter represents the center of gravity of all illuminated pixels within the ellipse.

In this case, the recognition of particles is performed according the following rule:

(a)if then the event is recognized as a gamma particle;

(b)if and deg, then the event is recognized as a gamma particle;

(c)otherwise, the event is rejected.

is a parameter which is adjusted according to the data set.

The major drawback of such approach is that the considered thresholds consist of constant values. Thus, a lack of flexibility is to be deplored. For example, it does not allow to take into consideration the various conditions of the experiment that may have a significant impact on the shape of signatures.

### 3.2. Intelligent Preprocessing

The second studied approach aims to make use of algorithms that already brought significant results in terms of pattern recognition. Neural networks are good candidates because they are a powerful computational model. On the other hand, their inherent parallelism makes them suitable for a hardware implementation. Although used in different fields of physics, these algorithms based on neural networks have successfully been implemented and have already proved their efficiency [5, 6]. Typical applications include particle recognition in tracking systems, event classification problems, off-line reconstruction of event, and online trigger in High-Energy Physics.

From the assumption that neural networks may be useful in such experiments, we have proposed a new Level 2 (L2) trigger system enabling to implement rather complex processing on the incoming images. The major issue with neural networks resides in the learning phase which strives to identify optimal parameters (weights) in order to solve the given problem. This is true when considering unsupervised learning in which representative patterns have to be iteratively presented to the network in a first learning phase until the global error has reached a predefined value.

One of the most important drawbacks of this type of algorithms is that the number of weights strongly depends on the dimensionality of the problem which is often unknown in practice. This implies to find the optimal structure of the network (number of neurons, number of layers) in order to solve the problem.

Moreover, the curse of dimensionality [7] constitutes another challenge when dealing with neural networks. This problem expresses a correlation between the size of the network and the number of examples to furnish. This relation is exponential, that is, if the network's size becomes significant, the number of training examples may become relatively huge. This cannot be considered in practice.

In order to reduce the size of the network, it is possible to simplify its, task that is, reduce the dimensionality of the problem. In this case, a preprocessing step aims at finding correlations on data and at applying basic transformations in order to ease the resolution. In this study, we advise to use an "intelligent" preprocessing based on the extraction of the intrinsic features of the incoming images.

#### 3.2.1. The Rejection Step

The rejection step has two significant roles. First, it aims to remove isolated pixels that are typically due to background. These pixels are eliminated by applying a filtering mask on the entire image in order to keep the only relevant information, that is, clusters of pixels. This consists in testing the neighborhood of each pixel of the image. As the image has an hexagonal mesh grid, a hexagonal neighborhood is used. The direct neighborhood of each pixel of the image is tested. If none of the neighbors are activated, the corresponding central pixel is considered as isolated and deactivated. Second, the rejection step permits to eliminate particles that cannot be distinguished by the classifier. Very small images ( pixels) are discarded since they contain poor information that cannot be deciphered.

#### 3.2.2. The Preprocessing Step

The envisaged system is based on a preprocessing step whose role consists in applying basic transformations on incoming images in order to isolate the main characteristics of a given image. The most important role of the preprocessing is to guarantee invariance in orientation (rotation and translation) of the incoming images. Since signatures of particles within the image depend on the impact point of an incident particle, the image may result in a series of pixels located wherever on the telescope. Without using a preprocessing stage based on orientation invariance, the 2048 inputs of the classifier would completely differ from an image to another although the basic shape of the particle would remain the same.

The retained preprocessing is based on the use of Zernike moments. These moments are mainly considered in shape reconstruction [8] and can be easily made invariant to changes in objects orientation. They are defined as a set of orthogonal functions based on complex polynomials originally introduced in [9]. Zernike polynomials can be expressed as

where , is a nonnegative integer, is apositive integer such as is even and , : length of a vector from the origin to a point such as , that is, where , : angle between the axis and the vector extending from the origin to a point .

: Zernike polynomial defined as:

Zernike moments are expressed according to

where refers to the pixels' value of coordinates(x,y). The rotation invariance property of Zernike moments is due to the intrinsic nature of such moments. In order to guarantee translation invariance as well, it is necessary to align the center of the object to the center of the unit circle. This may be performed by changing the coordinates and of each processing point by the coordinates and where and refer to the center of the signature and may be obtained by

In this case, is expressed as follows:

In the context of our application, it has been found that considering the first 8-order Zernike moments was sufficient to obtain the best performances. This implies to compute 25 polynomials for each of the pixels within an image. Then, it is necessary to accumulate these values in order to obtain 25 real values corresponding to all the Zernike moments of the image. The module of these moments is then computed and a normalization step is fulfilled in order to scale the obtained values within the −1 to 1 range. These values are then provided to the neural network.

#### 3.2.3. The Neural Classifier

According to the nature of the network, the value of the output may be computed according to (6).

In (6), represents the output; and respectively, represent the weights connecting the output layer and the hidden layer and the weights connecting the hidden layer and the input nodes. is the number of neurons in the hidden layer and is the number of inputs. denotes the value of an input node and is an activation function. In our case, the nonlinear function has been used:

In the considered application, the output layer is composed of a three neurons (which value ranges between −1 and 1) corresponding to the type of particle to identify. Each output refers to a gamma, proton, and muon particle, respectively. If the value of an output neuron is positive, it may be assumed that the corresponding particle has been identified by the network. In the case that more than one output neuron is activated, the maximum value is taken into account.

The learning phase has been performed off-line on a set of 4500 patterns computed on simulated images as the HESS2 telescope is not yet installed. The simulated images are generated thanks to series of Monte Carlo simulations. These patterns covered all ranges of energies and types of particles. 1500 patterns were considered for each class of particles. A previous study had determined the reliability of the patterns in order to consider the most representative patterns that may be collected by the telescope.

A classical backpropagation algorithm has been programmed off-line in order to get the optimal value of weights. The training have been performed simultaneously on two sets of patterns (learning and testing set). Once the error on the testing phase was minimum, the training was stopped ensuring that the weights had an optimal value.

The size of the input layer was determined according to the type of preprocessing that was envisaged. In the case of a Zernike preprocessing, this number has been set to 25 since it corresponds to the number of outputs furnished by the preprocessing step.

The number of hidden nodes (in the hidden layer) has been evaluated regarding the results obtained on a specific validation set of patterns. This precaution has been handled in order to ensure that the neural network was able to generalize on new data (i.e., it has not learnt explicitly).

### 3.3. Simulated Performances

Performances according to both approaches.

Gamma | Muon | Proton | |
---|---|---|---|

Hillas approach | 60% | 56% | 37% |

Neural approach | 95% | 58% | 41% |

According to Table 1, it may be seen that the neural solution provides significant improvement compared to classical methods in terms of classification. This improvement resides in the fact that a largest dimensionality of the problem has been taken into account. Whereas Hillas processing takes only five parameters into consideration, the number of inputs in the case of a neural preprocessing is set to 25. Moreover, as the Hillas approach only consists in applying strong "cuts" on predefined parameters, the neural approach is more flexible and guarantees nonlinear decision boundaries. It may be assumed that the considered neural network is capable of extracting the relevant information and discriminate between all images, efficiently. The major drawback of the neural approach is its relative complexity in terms of computation and hardware implementation. Although Hillas algorithms may be implemented in software, it is impossible to implement both the neural network and the preprocessing step in the same manner. In this context, dedicated circuits have to be designed in order to be compliant with the strong timing constraints imposed by the entire system. In our case, an L2-decision has to be taken at a rate of 3.5 KHz which corresponds to a timing constraint of 285 microseconds.

## 4. Hardware Implementation

The complete L2 trigger system is currently being built, making intensive use of the reconfigurable technology. Components such as FPGAs constitute an attractive alternative to classical circuits such as ASICs (Application Specific Integrated Circuits). This type of reconfigurable circuits tends to be more and more efficient in terms of speed and logic resources and is more and more envisaged in deeply constrained applications.

### 4.1. Hardware Implementation of Zernike Moments

Although very efficient, Zernike moments are known for their computation complexity. Many solutions have been proposed for the fast implementation of the Zernike moments. Some algorithms are based on recursivity [11], reuse of previous parts of the computation [12] or moment generators [13].

Since using a moment generator allows a reduction of the number of operations, we have decided to follow this approach, that is, to compute Zernike moments from accumulation moments.

#### 4.1.1. Zernike Moments via Accumulation Moments

The mechanism of a moment generator [14] can be summarized by the expression of the geometric moments with respect to the point of coordinates from the accumulation moments:

with being the accumulation moments of order , and being the pixels' values in the image and

According to (8), it is important to note that geometric moments may be expressed as a function of accumulation moments. In the context of our application, (10) to (23) demonstrate how to calculate the Zernike moments from the geometric moments and thus from accumulation moments.

We have seen that Zernike moments may be expressed as follows:

The expressions of and can be rewritten as

where are the coordinates of the image center computed as explained in (4):

In order to simplify the equations, we note and . In this case,

According to the binomial theorem, the development of a given polynom can be expressed as follows:

It is then possible to modify the following expressions:

Thus, (13) can be reformulated as follows:

The next step consists in considering the last point in the equation of Zernike moments with respect to the center of the image:

Since the coordinates of the pixels in the image are expressed as real numbers, we need to express these coordinates with integers in order to formulate the Zernike moments in function of the geometric moments. As we can see in Figure 7, the even rows have to be distinguished from the odd rows. Therefore, the coordinate is expressed in two different ways according to the type of row (even or odd row).

where and are positive integers such as and with corresponding to the number of columns, and corresponding to the number of rows. (resp., ) is the distance between two adjacent columns (resp., rows) and and correspond to the new position of the origin of the image in the upper left corner.

In the following equations, since the first part of the expressions does not change, the second part is just developed:

In this case, we propose to figure out the even and odd parts of the image, let if and if . In this case, the sums on will be bounded by and

Equation (23) shows that the Zernike moments can be computed from the geometric moments. If we consider two accumulation grids, the first computes the accumulation moments on the odd lines of the image and the second on the even lines. Since the computation is divided into two different parts, the image should be arranged in two components: the odd component of the image and the even one. Therefore, according to (8), the analogy gives an expression of the Zernike moments which is function of (accumulation moments computed from the odd component of the image) and (accumulation moments computed from the even component of the image) by setting and :

By reinjecting (24) in the (23), Zernike moments are reformulated as follows:

In an analogous way, the coordinates of the center of the image can be computed from the accumulation moments:

where

It comes

We have developed here an algorithm enabling the computation of Zernike moments based on the moment generator using the accumulation moments. This algorithm has the advantage to be used on images which have particular topologies since their mesh grid is regular or semiregular by the use of a second accumulation grid. The second advantage of this algorithm is its simplicity to be implemented on FPGA, for instance. The base of this algorithm relies on the accumulation moments and is easily computed thanks to a simple accumulation grid.

#### 4.1.2. Architecture Description

To make the exploitation of (25) easier, we need to reorder the terms to get an expression of the Zernike moments such as

where

The registers used between the column accumulators are synchronized at the end of each row; so their clock enable depends on the image topology. In our case, corners have been filled with zeros before dividing the image. Therefore, the size of each image's component is . In this case, the accumulation moment is computed on clock cycles from the moment when the first pixel arrives into the accumulation grid.

A Zernike computation block aims to compute the module of Zernike moments from the accumulation moments that are provided by the grids and from the module that furnishes the coefficients (see Figure 8). This block consists in summing the different coefficients and in computing the module of each moment. In order to reduce the amount of logical resources to provide, the computation of the square root is simplified according to the following approximation:

This approximation is often utilized in image processing and does not impact significantly the final results.

#### 4.1.3. FPGA Implementation of Zernike Moment's Computation

In order to compute the Zernike moment from the accumulation, we proposed an original architecture which is presented in Figure 10. This architecture is very regular and simplifies the implementation on an FPGA target. Furthermore, we can notice that the hardware required is simple to design for both the moments' accumulation and moments' computation. In fact, the computations are based on a multiplier and an adder. These constitute the MAC (for Multiply-ACcumulate) operator and are widely available in current FPGA devices. In order to improve performances, MAC operators are integrated in some FPGA devices as a hardwired component like DSP48 in Xilinx Virtex4.

Two implementation approaches are possible in which either hardware or time optimization is considered.

Hardware Optimization

Time Optimization

### 4.2. Hardware Implementation of the Neural Network

The parallel nature of neural networks makes them very suitable for hardware implementation. Several studies have been performed so far allowing complex configurations to be implemented in reconfigurable circuits [15, 16].

In this example, the neural architecture is implementing a 5-input MLP with 7 hidden nodes and 3 outputs. These parameters are easily modifiable since the proposed circuit is scalable.

Input data are accepted sequentially and applied to the series of multipliers. corresponds to the th input of the present state whereas corresponds to the th of the next set. Data arrive at each clock cycle.

At each clock cycle, at any particular level of adder, apart from the addition operation between the multiplier output and the sum from the previous level, the multiplication operation of the next set of inputs at the adjacent multiplier is also simultaneously performed. The sum, thus, ripples and accumulates through the central adders (48 bits) until it is fed to a barrel shifter that aims to translate the data into a 16-bit address. The obtained sum addresses a sigmoid block memory (SIGMOID0) containing 65536 values of 18 bits.

This block feeds the outputs of the hidden layer sequentially to three MAC units for the output layer calculation. Finally a multiplexer distributes serially the results of the output layer to another sigmoid block memory (SIGMOID1). After a study on data representation, it has been decided to code the incoming data in 18 bits. Weights are stored in ROM (Read-only Memories) containing 256 words of 18 bits. The control of the entire circuit is performed by a simple state machine that aims to organize the sequence of computations and memory management.

The number of multipliers required for the network is where is the number of inputs and is the number of outputs. Considering that the number of hidden nodes may be large compared to the number of inputs and the number of outputs, the adopted solution does not affect the number of multipliers which is a great relief. In this context, it is also important to note that the design is very easily scalable to accommodate more hidden, input or output nodes. For example, adding a hidden node does not impact the number of resources but requires an additional cycle of computation. Adding an input may be accommodated by the addition of another ROM, multiplier, and adder set to the series of adders at the centre (part HL of the figure). Moreover, the addition of an output node can be fulfilled by adding another ROM, MAC unit, and sigmoid block to the part OL of the figure.

Another advantage of the architecture is that a single activation function (sigmoid block) is required to compute the complete hidden layer. This block consists of a Look-up Table (LUT) that stores 65536 values of the function.

In general, the time required to obtain the outputs after the arrival of the first input is fixed to , where is the number of inputs, and is the number of hidden units. In every cycle, number of multiplications is performed ( is the number of output units).

## 5. Performances

The complete architecture (preprocessing + neural network) has been implemented in a Xilinx Virtex4 (xc4lx100) FPGA which is the part that has been retained for the trigger implementation. This type of reconfigurable circuit exhibits a lot of dedicated resources such as memory blocks or DSP blocks that allow to compute a MAC very efficiently.

### 5.1. Resources Requirements

Summary of occupied resources.

Module | Number of used logic slices/ | Used DSP blocks/ | Number of used memory bits/ |
---|---|---|---|

available | available | available (Kb) | |

Accumulation moments | 1786/49152 | 0/96 | 0 /4320 |

Zernike moments | 75/49152 | 60/96 | 21/4320 |

Neural Network | 477/49152 | 28/96 | 2808/4320 |

Total | 2338/49152 (4%) | 88/96 (92%) | 2829 /4320 (65.5%) |

Concerning the hardware implementation of the neural network, it is important to notice that, independently of the configuration, the amount of used resources is very low. Nevertheless, one may deplore an important usage of memory blocks destined to store the values of the sigmoid functions. This issue may be circumvented in case where hardware resources constitute an issue. A modified activation function could be used [17]. This has a shape quite similar to the sigmoid function and is very easy to implement on hardware with just a number of shifts and adds. This function can be executed with an error less than

According to Table 3, it is clear that the entire system fits in an FPGA without consuming to much logic (4%). Moreover, the complete architecture has been devised in order to take full benefit of the intrinsic dedicated resources of the FPGA, that is, DSP and memory blocks.

### 5.2. Timing

It is important to note that most of the computation time is monopolized by the computation of Zernike moments from the accumulation moments. This is mainly due to the fact that the number of accumulations to perform is huge (104663 accumulations for an order-8) and that these computations are performed iteratively. Even if we have decided to parallelize the architecture in five stages, the number of iterations remains high ( ). A current work is performed to optimize the computations in this block for further improvements.

The maximum clock frequency has been estimated at 120 MHz and 366 MHz for the DSP blocks.

## 6. Conclusion

In this article, we have presented an original solution that may be seen as an intelligent way of triggering data in the HESS Phase-II experiment. The system relies on the utilization of image processing algorithms in order to increase the trigger efficiency. The hardware implementation has represented a challenge because of the relatively strong timing constraints 285 microseconds to process all algorithms. This problem has been circumvented by taking advantage of the nature of the algorithms. All these concepts are implemented making intensive use of FPGA circuits which are interesting for several reasons. First, the current advances in reconfigurable technology make FPGAs an attractive alternative compare to very powerful circuits such as ASICs. Moreover, their relatively small cost permits to rapidly implement a prototype design without major developmental constraints. The reconfigurability also constitutes a major point. It allows to configure the whole system according to the application needs, enabling flexibility and adaptivity. For example, in the context of the HESS project, it may be conceivable to reconfigure the chip according to the surrounding noise or to deal with specific experimental conditions.

## Authors’ Affiliations

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